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          <TD align=middle><FONT size=3>1997年10月托福閱讀全真試題 </FONT></TD></TR>
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          <TD class=l17><FONT class=f14 id=zoom></O:P></SPAN>
            <P></P>
            <P class=MsoNormal><SPAN lang=EN-US>Question 39-50<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal><SPAN lang=EN-US><SPAN 
            style="mso-spacerun: yes">&nbsp; </SPAN>Galaxies are the major 
            building blocks of the universe. A&nbsp;<BR>galaxy is giant family 
            of many millions of stars, and it is held&nbsp;<BR>together by its 
            own gravitational field. Most of the material&nbsp;<BR>universe is 
            organized into galaxies of stars together with&nbsp;<BR>gas and 
            dust.<O:P> </O:P></SPAN></P>
            <P class=MsoNormal><SPAN lang=EN-US><SPAN 
            style="mso-spacerun: yes">&nbsp; </SPAN>There are three main types 
            of galaxy: spiral, elliptical,&nbsp;<BR>and irregular. The Milky Way 
            is a spiral galaxy, a flattish disc&nbsp;<BR>of stars with two 
            spiral arms emerging from its central nucleus.&nbsp;<BR>About 
            one-quarter of all galaxies have this shape. 
            Spiral&nbsp;<BR>galaxies are well supplied with the interstellar gas 
            in which&nbsp;<BR>new stars form: as the rotating spiral pattern 
            sweeps around&nbsp;<BR>the galaxy it compresses gas and dust, 
            triggering the formation&nbsp;<BR>of bright young stars and in its 
            arms. The elliptical galaxies have a&nbsp;<BR>symmetrical elliptical 
            or spheroidal shape with no obvious&nbsp;<BR>structure. Most of 
            their member stars are very old and since&nbsp;<BR>ellipticals are 
            devoid of interstellar gas, no new stars are forming&nbsp;<BR>in 
            them. The biggest and brightest galaxies in the 
            universe&nbsp;<BR>are ellipticals with masses of about 1013 times 
            that of the Sun,&nbsp;<BR>these giants may frequently be sources of 
            strong radio&nbsp;<BR>emission, in which case they are called radio 
            galaxies. About two-<BR>thirds of all galaxies are elliptical. 
            Irregular galaxies comprise&nbsp;<BR>about one-tenth of all galaxies 
            and they come in many&nbsp;<BR>subclasses.<O:P> </O:P></SPAN></P>
            <P class=MsoNormal><SPAN lang=EN-US><SPAN 
            style="mso-spacerun: yes">&nbsp; </SPAN>Measurement in space is 
            quite different from measure-<BR>ment on Earth. Some terrestrial 
            distances can be expressed as&nbsp;<BR>intervals of time, the time 
            to fly from one continent to another&nbsp;<BR>or the time it takes 
            to drive to work, for example. By comparison&nbsp;<BR>with these 
            familiar yardsticks, the distances to the&nbsp;<BR>galaxies are 
            incomprehensibly large, but they too are made&nbsp;<BR>more 
            manageable by using a time calibration, in this case 
            the&nbsp;<BR>distance that light travels in one year. On such a 
            scale the&nbsp;<BR>nearest giant spiral galaxy, the Andromeda 
            galaxy, is two&nbsp;<BR>million light years away. The most distant 
            luminous objects seen&nbsp;<BR>by telescopes are probably ten 
            thousand million light years&nbsp;<BR>away. Their light was already 
            halfway here before the Earth&nbsp;<BR>even formed. The light from 
            the nearby Virgo galaxy set out&nbsp;<BR>when reptiles still 
            dominated the animal world.<O:P> &nbsp;<O:P> </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>39.The word "major" in line 1 is closest in meaning 
            to<O:P> &nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>intense<O:P> &nbsp;<BR>(B)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>principal<O:P> 
            &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>huge<O:P> 
            &nbsp;<BR>(D)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>unique<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>40.What does the second paragraph mainly discuss?<O:P> 
            &nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>The Milky 
            Way<O:P> &nbsp;<BR>(B)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>Major categories of galaxies<O:P> &nbsp;<BR>(C)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>How elliptical galaxies are 
            formed<O:P> &nbsp;<BR>(D)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>Differences between irregular and spiral galaxies<O:P> 
            </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>41.The word "which" in line 10 refers to 
            <O:P>&nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>dust<O:P> &nbsp;<BR>(B)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>gas<O:P> &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>pattern<O:P> &nbsp;<BR>(D)<SPAN style="mso-tab-count: 1"> 
            </SPAN>galaxy<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>42.According to the passage, new stars are formed in 
            spiral galaxies due to <O:P>&nbsp;<BR>(A)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>an explosion of gas<O:P> 
            &nbsp;<BR>(B)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>the 
            compression of gas and dust<O:P> &nbsp;<BR>(C)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>the combining of old 
            stars<O:P> &nbsp;<BR>(D)<SPAN style="mso-tab-count: 1"> 
            </SPAN>strong radio emissions<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>43.The word "symmetrical" in line 14 is closest in 
            meaning to<O:P> &nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>proportionally balanced<O:P> &nbsp;<BR>(B)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>commonly seen<O:P> 
            &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>typically 
            large<O:P> &nbsp;<BR>(D)<SPAN style="mso-tab-count: 1"> 
            </SPAN>steadily growing<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>44.The word "obvious" in line 14 is closest in meaning 
            to<O:P> &nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>discovered<O:P> &nbsp;<BR>(B)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>apparent<O:P> 
            &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>understood<O:P> &nbsp;<BR>(D)<SPAN style="mso-tab-count: 1"> 
            </SPAN>simplistic<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>45.According to the passage, which of the following is 
            NOT true of elliptical galaxies?<O:P> &nbsp;<BR>(A)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>They are the largest 
            galaxies.<O:P> &nbsp;<BR>(B)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>They mostly contain old stars.<O:P> &nbsp;<BR>(C)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>They contain a high amount of 
            interstellar gas.<O:P> &nbsp;<BR>(D)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>They have a spherical 
            shape.<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>46.Which of the following characteristics of radio 
            galaxies is mentioned in the passage?<O:P> &nbsp;<BR>(A)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>They are a type of elliptical 
            galaxy.<O:P> &nbsp;<BR>(B)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>They are usually too small to be seen with a telescope.<O:P> 
            &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>They are 
            closely related to irregular galaxies.<O:P> &nbsp;<BR>(D)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>They are not as bright as 
            spiral galaxies.<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>47.What percentage of galaxies are irregular?<O:P> 
            &nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>10%<O:P> 
            &nbsp;<BR>(B)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>25%<O:P> 
            &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>50%<O:P> 
            &nbsp;<BR>(D)<SPAN style="mso-tab-count: 1"> </SPAN>75%<O:P> 
            </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>48.The word "they" in line 29 refers to<O:P> 
            &nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>intervals<O:P> &nbsp;<BR>(B)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>yardsticks<O:P> 
            &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>distances<O:P> &nbsp;<BR>(D)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>galaxies<O:P> </SPAN><SPAN 
            lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>49.Why does the author mention the Virgo galaxy and the 
            Andromeda galaxy in the third paragraph?<O:P> &nbsp;<BR>(A)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>To describe the effect that 
            distance has no visibility.<O:P> &nbsp;<BR>(B)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>To compare the ages of two 
            relatively young galaxies.<O:P> &nbsp;<BR>(C)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>To emphasize the vast 
            distances of the galaxies from Earth.<O:P> &nbsp;<BR>(D)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>To explain why certain 
            galaxies cannot be seen by a telescope.<O:P> </SPAN><SPAN lang=EN-US 
            style="FONT-FAMILY: 宋體; mso-hansi-font-family: 'Times New Roman'">&nbsp;<O:P> 
            </O:P></SPAN></P>
            <P class=MsoNormal 
            style="MARGIN-LEFT: 12pt; TEXT-INDENT: -12pt; tab-stops: 12.0pt"><SPAN 
            lang=EN-US>50.The word "dominated" in line 37 is closest in meaning 
            to<O:P> &nbsp;<BR>(A)<SPAN style="mso-tab-count: 1">&nbsp; 
            </SPAN>threatened<O:P> &nbsp;<BR>(B)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>replaced<O:P> 
            &nbsp;<BR>(C)<SPAN style="mso-tab-count: 1">&nbsp; </SPAN>were 
            developing in<O:P> &nbsp;<BR>(D)<SPAN 
            style="mso-tab-count: 1">&nbsp; </SPAN>were prevalent in<O:P> 
            </SPAN></P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></O:P></FONT></TD></TR></TBODY></TABLE></TD></TR></TBODY></TABLE>
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